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TU=ℏa/(2πckB)∼3×103 KT_U = \hbar a/(2\pi c k_B) \sim 3\times10^3\,\mathrm K

Why this formula appears here

Electrons circulating in a storage ring undergo enormous proper acceleration — for an ultra-relativistic beam of Lorentz factor γ\gamma on a ring of radius r , the proper centripetal acceleration is a ≈\approx γ2\gamma^2 c2c^2/r . For beam parameters typical of a large electron-positron collider, with γ\gamma of order 2×\times10^5 and r of order several kilometers, this works out to a ∼\sim 8×\times10^{23}\,m s−2\mathrm{m\,s^{-2}} , corresponding by the Unruh formula to TUT_U = ℏ\hbar a/(2π\pi c kBk_B) ∼\sim 3×\times10^3\,K\mathrm K — a temperature scale that is, remarkably, not astronomically small, unlike the roughly 10^{-19}\,K\mathrm K an Earth-bound laboratory accelerometer would need a planet’s worth of…

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TU=ℏa/(2πckB)∼3×103 KT_U = \hbar a/(2\pi c k_B) \sim 3\times10^3\,\mathrm K

Equation 105 · Evolutionary Physics

No Particle Without a Cosigner

This equation states an equality: the expressions on both sides have the same value under the article’s assumptions.

Electrons circulating in a storage ring undergo enormous proper acceleration — for an ultra-relativistic beam of Lorentz factor γ\gamma on a ring of radius r , the proper centripetal acceleration is a ≈\approx γ2\gamma^2 c2c^2/r . For beam parameters typical of a large electron-positron collider, with γ\gamma of order 2×\times10^5 and r of order several kilometers, this works out to a ∼\sim 8×\times10^{23}\,m s−2\mathrm{m\,s^{-2}} , corresponding by the Unruh formula to TUT_U = ℏ\hbar a/(2π\pi c kBk_B) ∼\sim 3×\times10^3\,K\mathrm K — a temperature scale that is, remarkably, not astronomically small, unlike the roughly 10^{-19}\,K\mathrm K an Earth-bound laboratory accelerometer would need a planet’s worth of…

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